大质量比双黑洞给数值相对论带来的挑战课件.ppt
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- 质量比 黑洞 数值 相对论 带来 挑战 课件
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1、Port AMSS-NCKU code to GPU Zhoujian Cao Academy of Mathematics and System Science,CAS Cowork with Zhihui Du,Steven Brandt,Frank Loeffler and Quan Yang 2013-8-72013 International School on Numerical Relativity and Gravitational Waves,Pohang KoreaOutline Motivations from gravitational wave detection N
2、ew parallel mesh refinement numerical scheme GPU acceleration for NR SummaryThe most stringent test of GR the anomalous precession of the perihelion of Mercury(1915,v )Deflection of Starlight(1919,v )gravitational redshift (1965,v )gravitational time delay effect(1968,v )Evidence of Gravitational Wa
3、ves(1978,v )frame-dragging effect(2010,v )Direct gravitational wave detection(?,v1)1010710104GR=Newtonian Gravity+PN(v)+PN(v2)+101076107101076102Gravitational wave astronomy Search back to extremely early universe Hear the dark universe Gravitational wave and its detectionCategory of Black Holes Sup
4、er massive black hole:M:105109 Msun Stellar massive black hole:M:1-10s Msun Intermediate massive black hole:M:10s105 Msun(mainly in globular cluster)Farrell,et al,Nature 460(2009)73;Feng,et al,New Astronomy Reviews 55(2011)166Category of Black Holes BinaryIMBHALIAXuefei Gong,et al,CQG 28,094012(2011
5、)1:10001:1Advanced LIGOAbadie,et al,PRD 85,102004(2012)IMBH and GW detectionData analysis and templateRef to Sang Hoon Ohs lectureTemplate model for BBH?Yi Pans talk,2013Template model for BBH PN templates:for early stage of inspiralling EOBNR(effective one body model together with numerical relativ
6、ity):for full inspiral+merger+ring down stage;works well for mass ratio less than 1:8 and extreme mass ratio BBH,high spinning,precession!But no reliable template for mass ratio 1:10 to 1:100From a given separation of the two BHs,when mass ratio increases the number of orbit increases quickly.This r
7、equires that the numerical simulation with full GR increases much consequently.In contrast to 1:1,1:100 needs 10 times more computation cost.PN estimationComputational cost1:1,9 days1:100,20 daysLSSC cluster II,128 CPUs,for last 2 orbits computational cost 1 to 20!Challenge of large mass BBH to NR C
8、ompared to 1:1,the computational cost of 1:100 BBH increase roughly 200 times!For typical simulation of 1:1 BBH,14 days are needed.So by straight forward method to 1:100,roughly 1year is needed!Possible ways out 1.Physical level:approximation method,such as self force frame work(but still first orde
9、r yet),2.Numerical Algorithm level:implicit scheme R.Lau et al,PRD 84,084023(2011),combine Cauchy evolution to null evolution,3.Computer level:improve scalability to use more CPUs,use GPU,Possible ways out 1.Physical level:approximation method,such as self force frame work(but still first order yet)
10、,2.Numerical Algorithm level:implicit scheme R.Lau et al,PRD 84,084023(2011),combine Cauchy evolution to null evolution,3.Computer level:improve scalability to use more CPUs,use GPU,Mesh refinement schemeHigh resolution mesh grids for region near BH,while low resolution mesh grids for far regionMesh
11、 refinement in CFDResult based on PARAMESHPARAMESHGrACEJASMINComparison of NR and CFD NR(only for BH):computational expensive on single grid point,but functions quite smooth few grid points(handrads),high order finite difference CFD:computation on single point is cheap,but fluid dynamics quite compl
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